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Oblate Schwarzschild approximation for polarized radiation from rapidly rotating neutron stars

Oblate Schwarzschild approximation for polarized radiation from rapidly rotating neutron stars

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2444451567

Oblate Schwarzschild approximation for polarized radiation from rapidly rotating neutron stars

About this item

Full title

Oblate Schwarzschild approximation for polarized radiation from rapidly rotating neutron stars

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2020-09

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

We have developed a complete theory for the calculation of the observed Stokes parameters for radiation emitted from the surface of a rapidly rotating neutron star (NS) using the oblate Schwarzschild approximation. We accounted for the rotation of the polarization plane due to relativistic effects along the path from the stellar surface to the obse...

Alternative Titles

Full title

Oblate Schwarzschild approximation for polarized radiation from rapidly rotating neutron stars

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2444451567

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2444451567

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2009.08852

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